BD-03_5215: found in 2 paper(s).

Labels:

/D.L.Burris et al.(2000)/ /B.W.Carney et al.(2003)/

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A0014

Title NEUTRON-CAPTURE ELEMENTS IN THE EARLY GALAXY: INSIGHTS FROM A LARGE SAMPLE OF METAL-POOR GIANTS
ADS D.L.Burris et al.,ApJ, 544, 302, 2000
Authors D. L. Burris, C. A. Pilachowski, T. E. Armandroff, C. Sneden, J. J. Cowan, H. Roe

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A N/A MAYALLKPNO 20000 100-200 N/A N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Atmospheric data

Teff 5700
log g 2.80
vturb 1.80

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Fe...-1.16...6.34
Ba...-0.700.461.43
Eu...-0.600.56-0.09
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)


A0138

Title Spectroscopic Binaries, Velocity Jitter, and Rotation in Field Metal-poor Red Giant and Red Horizontal-Branch Stars
ADS B.W.Carney et al.,AJ, 125, 293, 2003
Authors B. W. Carney, D. W. Latham, R. P. Stefanik, J. B. Laird, J. A. Morse

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A 2445931.72998 WYETH N/A N/A N/A -294.70+-1.07
N/A 2445952.64177 WYETH N/A N/A N/A -293.55+-0.79
N/A 2446275.72932 WYETH N/A N/A N/A -292.92+-0.62
N/A 2446607.75952 WYETH N/A N/A N/A -292.64+-1.60
N/A 2446687.63046 WYETH N/A N/A N/A -294.15+-0.77
N/A 2446993.78504 WYETH N/A N/A N/A -293.02+-0.72
N/A 2447347.88044 WYETH N/A N/A N/A -293.85+-0.57
N/A 2447734.71134 WYETH N/A N/A N/A -294.00+-0.70
N/A 2448783.82590 WYETH N/A N/A N/A -293.42+-0.86
N/A 2449144.95804 TILLINGHAST N/A N/A N/A -293.99+-0.54
N/A 2450640.79712 WYETH N/A N/A N/A -293.74+-0.65
N/A 2450671.75629 WYETH N/A N/A N/A -294.66+-0.61
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination -030740
Right Ascension 212801.3

Binarity

Vrad -293.73

Photometric data

V-R 0.598
V-K 1.82

Atmospheric data

Teff 5420
log g 2.6

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Fe...-1.64...5.86
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)